The Star Formation Rate Intensity Distribution Function: Implications for the Cosmic Star Formation Rate History of the Universe
The Astrophysical Journal2002Vol. 570(2), pp. 492–501
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Abstract
We address the effects of cosmological surface brightness dimming on observations of faint galaxies by examining the distribution of “unobscured ” star formation rate intensities versus redshift. We use the star formation rate intensity distribution function to assess the ultraviolet luminosity density versus redshift, based on our photometry and photometric redshift measurements of faint galaxies in the HDF and the HDF–S WFPC2 and NICMOS fields. We find 1 Based on observations with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope
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